KM López
Discovery and analysis of a ULX nebula in NGC 3521★
López, KM; Jonker, PG; Heida, M; Torres, MAP; Roberts, TP; Walton, DJ; Moon, D-S; Harrison, FA
Authors
PG Jonker
M Heida
MAP Torres
Professor Tim Roberts t.p.roberts@durham.ac.uk
Professor
DJ Walton
D-S Moon
FA Harrison
Abstract
We present Very Large Telescope/X-shooter and Chandra X-ray observatory/ACIS observations of the ULX [SST2011] J110545.62+000016.2 in the galaxy NGC 3521. The source identified as a candidate near-infrared counterpart to the ULX in our previous study shows an emission line spectrum of numerous recombination and forbidden lines in the visible and near-infrared spectral regime. The emission from the candidate counterpart is spatially extended (∼34 pc) and appears to be connected with an adjacent H II region, located ∼138 pc to the NE. The measured velocities of the emission lines confirm that both the candidate counterpart and H II region reside in NGC 3521. The intensity ratios of the emission lines from the ULX counterpart show that the line emission originates from the combined effect of shock and photoionisation of low metallicity (12 + log (O/H) = 8.19 ± 0.11) gas. Unfortunately, there is no identifiable spectral signature directly related to the photosphere of the mass-donor star in our spectrum. From the archival Chandra data, we derive the X-ray luminosity of the source in the 0.3–7 keV range to be (1.9 ± 0.8) × 1040 erg cm−2 s−1, almost a factor of four higher than what is previously reported.
Citation
López, K., Jonker, P., Heida, M., Torres, M., Roberts, T., Walton, D., …Harrison, F. (2019). Discovery and analysis of a ULX nebula in NGC 3521★. Monthly Notices of the Royal Astronomical Society, 489(1), 1249-1264. https://doi.org/10.1093/mnras/stz2127
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 29, 2019 |
Online Publication Date | Aug 5, 2019 |
Publication Date | Oct 31, 2019 |
Deposit Date | Aug 13, 2019 |
Publicly Available Date | Aug 13, 2019 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 489 |
Issue | 1 |
Pages | 1249-1264 |
DOI | https://doi.org/10.1093/mnras/stz2127 |
Related Public URLs | https://arxiv.org/pdf/1907.12814.pdf |
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Copyright Statement
This article has been accepted for publication in the Monthly notices of the Royal Astronomical Society ©: 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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